Guide field dependence of energy spectrum and energy transfer in reconnection

Authors: Michael Shay(University of Delaware), Tulasi N. Parashar (Victoria University of Wellington), William H. Matthaeus (University of Delaware) Classic picture of magnetic reconnection has shownView More

SOFIE (Solar-wind with Field-lines and Energetic-particles): A data-driven and self-consistent SEP modeling and forecasting tool

Authors: Lulu Zhao (University of Michigan), Igor Sokolov (University of Michigan), Tamas Gombosi (University of Michigan), Zhenguang Huang (University of Michigan), Gabor Toth (University ofView More

Acceleration of Solar Energetic Particles (SEPs) through a CME-driven Shock and Streamer Interaction

Authors: Matthew West (Southwest Research Institute), Federica Frassati (National Institute of Astrophysics – Astrophysical Observatory of Turin), Monica Laurenza (Istituto di Astrofisica e Planetologia Spaziali),View More

Modeling the Solar Wind During Different Phases of the Last Solar Cycle

Authors: Gabor Toth (University of Michigan), Nishtha Sachdeva (University of Michigan), Lulu Zhao (University of Michigan), Bart van der Holst (University of Michigan), Igor SokolovView More

Advantages of Characterising the Suprathermal Electrons Pitch-angle Distribution

Authors: Fernando Carcaboso (NASA Goddard Space Flight Center, The Catholic University of America), Raúl Gómez-Herrero (Space Research Group, University of Alcalá), Francisco Espinosa Lara (SpaceView More

Quantifying the Impacts of Interplanetary Propagation and Transient Events on Solar Energetic Particle Intensity-Time Profiles

Authors: Alicia K. Petersen (Air Force Research Lab, NRC), Stephen M. White (Air Force Research Lab, Kirtland AFB), Stephen W. Kahler (Air Force Research Lab,View More

The Variation of the Pitch-angle Distribution of 500 MeV solar protons at 1 au in a Weak Pitch-angle Scattering and in the Large-scale Turbulent Interplanetary Magnetic Field

Authors: Ashraf Moradi (University of Arizona), Joe Giacalone (University of Arizona) Solar protons with rigidities higher than 1 GV (432 MeV) penetrate Earth’s atmosphere, generateView More

The First Absolute Brightness Measurements and MHD Model Predictions of Fe X, XI, and XIV out to 3.4 Rs

Authors: Benjamin Boe (NSF Postdoctoral Fellow. Institute for Astronomy, University of Hawaii), Shadia Habbal (Institute for Astronomy, University of Hawaii), Cooper Downs (Predictive Science Inc.),View More

Mapping the Sun’s Far-Side Magnetic Flux from Near-side Helioseismic Measurements by Deep Learning

Authors: Ruizhu Chen (Stanford University), Junwei Zhao (Stanford University), Shea A. Hess Webber (Stanford) The Sun’s far-side magnetic field is important for space weather forecastingView More

Understanding Atmospheric Absorption Effects on UV Spectra from Sounding Rockets using a Spherical-Shells Model

Authors: Nicolas Donders (The University of Alabama in Huntsville, Department of Space Science and The Center for Space Plasma and Aeronomic Research), Amy Winebarger (NASAView More

Exploring the Corona With the Newest Coronagraph at the Mauna Loa Solar Observatory (MLSO)

Authors: Joan Burkepile (High Altitude Observatory HAO), Steven Tomczyk (HAO), Ben Berkey (HAO), Marc Cotter (HAO) , Michael Galloy (HAO), Sarah Gibson (HAO), Don KolinskiView More

Integrating automated coronal mass ejection detection alerts from a ground based coronagraph for use in solar energetic particle event forecasting

Authors: M. D. Galloy (HAO Boulder, CO), J. T. Burkepile (HAO Boulder, CO), M. L. Mays (NASA GSFC), J. T. Jones (NASA GSFC), O. C.View More

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